Relative fragmentation in ternary systems within the temperature-dependent relativistic mean-field approach

M. T. Senthil Kannan, Bharat Kumar, M. Balasubramaniam, B. K. Agrawal, and S. K. Patra
Phys. Rev. C 95, 064613 – Published 22 June 2017

Abstract

For the first time, we apply the temperature-dependent relativistic mean-field (TRMF) model to study the ternary fragmentation of heavy nuclei using the level density approach. The relative fragmentation probability of a particular fragment is obtained by evaluating the convolution integrals that employ the excitation energy and the level density parameter for a given temperature calculated within the TRMF formalism. To illustrate, we have considered the ternary fragmentations in Cf252, Pu242, and U236 with a fixed third fragment A3=Ca48, O20, and O16, respectively. The relative fragmentation probabilities are studied for the temperatures T=1, 2, and 3 MeV. For the comparison, the relative fragmentation probabilities are also calculated from the single-particle energies of the finite range droplet model (FRDM). In general, the larger phase space for the ternary fragmentation is observed indicating that such fragmentations are most probable ones. For T=2 and 3 MeV, Sn+Ni+Ca is the most probable combination for the nucleus Cf252. However, for the nuclei Pu242 and U236, the maximum fragmentation probabilities at T=2 MeV differ from those at T=3 MeV. For T=3 MeV, the closed shell (Z=8) light-mass fragment with its corresponding partners has larger scission point probabilities. But, at T=2 MeV, Si, P, and S are favorable fragments with the corresponding partners. It is noticed that the symmetric binary fragmentation along with the fixed third fragment for Pu242 and U236 is also favored at T=1 MeV.

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  • Received 30 November 2016
  • Revised 15 May 2017

DOI:https://doi.org/10.1103/PhysRevC.95.064613

©2017 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

M. T. Senthil Kannan1,*, Bharat Kumar2,3, M. Balasubramaniam1, B. K. Agrawal3,4, and S. K. Patra2,3,†

  • 1Department of Physics, Bharathiar University, Coimbatore 641046, India
  • 2Institute of Physics, Sachivalaya Marg, Bhubaneswar 751005, India
  • 3Homi Bhabha National Institute, Anushakti Nagar, Mumbai 400094, India
  • 4Saha Institute of Nuclear Physics, 1/AF, Bidhannagar, Kolkata 700064, India

  • *senthilthulasiram@gmail.com
  • patra@iopb.res.in

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Issue

Vol. 95, Iss. 6 — June 2017

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